The infancy of core-collapse supernova remnants

Abstract

We present 3D hydrodynamic simulations of neutrino-driven supernovae (SNe) with the PROMETHEUS-HOTB code, evolving the asymmetrically expanding ejecta from shock breakout until they reach the homologous expansion phase after roughly one year. Our calculations continue the simulations for two red supergiant (RSG) and two blue supergiant (BSG) progenitors by Wongwathanarat et al., who investigated the growth of explosion asymmetries produced by hydrodynamic instabilities during the first second of the explosion and their later fragmentation by Rayleigh-Taylor instabilities. We focus on the late time acceleration and inflation of the ejecta caused by the heating due to the radioactive decay of ${}^{56}$Ni to ${}^{56}$Fe and by a new outward-moving shock, which forms when the reverse shock from the He/H-shell interface compresses the central part of the ejecta. The mean velocities of the iron-rich ejecta increase between 100 km/s and 350 km/s ($\sim$8-30\%), and the fastest one percent of the iron accelerates by up to $\sim$1000 km/s ($\sim$20-25\%). This 'Ni-bubble effect', known from 1D models, accelerates the bulk of the nickel in our 3D models and causes an inflation of the initially overdense Ni-rich clumps, which leads to underdense, extended fingers, enveloped by overdense skins of compressed surrounding matter. We also provide volume and surface filling factors as well as a spherical harmonics analysis to characterize the spectrum of Ni-clump sizes quantitatively. Three of our four models give volume filling factors larger than 0.3, consistent with what is suggested for SN 1987A by observations.

arXiv comment30 pages, 22 figures, 6 tables, extended discussion of correlation of late and initial explosion asymmetries, accepted by MNRAS

References in corpus (84)

• Stability of Standing Accretion Shocks, With an Eye Toward Core Collapse Supernovae
• On the Nature of Core Collapse Supernova Explosions
• A two-parameter criterion for classifying the explodability of massive stars by the neutrino-driven mechanism
• The "Yin-Yang Grid": An Overset Grid in Spherical Geometry
• Multidimensional Supernova Simulations with Approximative Neutrino Transport I. Neutron Star Kicks and the Anisotropy of Neutrino-Driven Explosions in Two Spatial Dimensions
• Non-spherical Core Collapse Supernovae I. Neutrino-Driven Convection, Rayleigh-Taylor Instabilities, and the Formation and Propagation of Metal Clumps
• Three-dimensional neutrino-driven supernovae: Neutron star kicks, spins, and asymmetric ejection of nucleosynthesis products
• Young core collapse supernova remnants and their supernovae
• Three-dimensional core-collapse supernova simulated using a 15 $M_{\odot }$ progenitor
• Asymmetries in core-collapse supernovae from maps of radioactive ${}^{44}$Ti in CassiopeiaA
• Supernova Simulations from a 3D Progenitor Model -- Impact of Perturbations and Evolution of Explosion Properties
• Three-Dimensional Simulations of Core-Collapse Supernovae: From Shock Revival to Shock Breakout
• Instability of a stalled accretion shock: evidence for the advective-acoustic cycle
• Neutrino-driven explosion of a 20 solar-mass star in three dimensions enabled by strange-quark contributions to neutrino-nucleon scattering
• A Comparison of Two- and Three-dimensional Neutrino-hydrodynamics simulations of Core-collapse Supernovae
• Nucleosynthesis-relevant conditions in neutrino-driven supernova outflows. I. Spherically symmetric hydrodynamic simulations
• Three-Dimensional Simulations of Mixing Instabilities in Supernova Explosions
• Exploring Fundamentally Three-dimensional Phenomena in High-fidelity Simulations of Core-collapse Supernovae
• Neutrino-driven supernova of a low-mass iron-core progenitor boosted by three-dimensional turbulent convection
• The Spherical Accretion Shock Instability in the Linear Regime
• Multidimensional supernova simulations with approximative neutrino transport. II. Convection and the advective-acoustic cycle in the supernova core
• A Successful 3D Core-Collapse Supernova Explosion Model
• Massive Stars in the Range $13-25{\mathrm{M}}_{\odot }$: Evolution and Nucleosynthesis. II. the Solar Metallicity Models
• Numerical Analysis on Standing Accretion Shock Instability with Neutrino Heating in the Supernova Cores
• The Three-Dimensional Structure of Cassiopeia A
• Production and Distribution of ${}^{44}$Ti and ${}^{56}$Ni in a Three-dimensional Supernova Model Resembling Cassiopeia A
• General Relativistic Three-Dimensional Multi-Group Neutrino Radiation-Hydrodynamics Simulations of Core-Collapse Supernovae
• Three-Dimensional Supernova Explosion Simulations of 9-, 10-, 11-, 12-, and 13-M${}_{\odot }$ Stars
• Non-Spherical Core-Collapse Supernovae II. Late-Time Evolution of Globally Anisotropic Neutrino-Driven Explosions and Implications for SN 1987A
• Three-dimensional Models of Core-collapse Supernovae From Low-mass Progenitors With Implications for Crab
• The Progenitor Dependence of Three-Dimensional Core-Collapse Supernovae
• The distribution of radioactive ${}^{44}$Ti in Cassiopeia A
• Gamma-Ray Transfer and Energy Deposition in Supernovae
• Progenitor-dependent Explosion Dynamics in Self-consistent, Axisymmetric Simulations of Neutrino-driven Core-collapse Supernovae
• A Detailed Kinematic Map of Cassiopeia A's Optical Main Shell and Outer High-Velocity Ejecta
• Hydrodynamical Neutron Star Kicks in Three Dimensions
• The Nucleosynthetic Imprint of 15-40 Solar Mass Primordial Supernovae on Metal-Poor Stars
• Direct Confirmation of the Asymmetry of the Cas A Supernova with Light Echoes
• Modeling SNR Cassiopeia A from the Supernova Explosion to its Current Age: The role of post-explosion anisotropies of ejecta
• Non-radial instabilities of isothermal Bondi accretion with a shock: vortical-acoustic cycle vs post-shock acceleration
• The Spiral Modes of the Standing Accretion Shock Instability
• Simulating Self-gravitating Hydrodynamic Flows
• Mixing in Zero and Solar Metallicity Supernovae
• The First Second of a Type-II Supernova: Convection, Accretion, and Shock Propagation
• High angular resolution ALMA images of dust and molecules in the SN 1987A ejecta
• Hydrodynamical Neutron-star Kicks in Electron-capture Supernovae and Implications for the CRAB Supernova
• The Bubble-like Interior of the Core-Collapse Supernova Remnant Cassiopeia A
• Revival of the Fittest: Exploding Core-Collapse Supernovae from 12 to 25 M${}_{\odot }$
• Multi-D Simulations of Ultra-Stripped Supernovae to Shock Breakout
• The fully developed remnant of a neutrino-driven supernova: Evolution of ejecta structure and asymmetries in SNR Cassiopeia A
• Aspherical Core-Collapse Supernovae in Red Supergiants Powered by Nonrelativistic Jets
• Gamma-Ray Lines from Asymmetric Supernovae
• On the photometric and spectroscopic diversity of Type II supernovae
• High Ratio of 44Ti/56Ni in Cas A and Axisymmetric Collapse-Driven Supernova Explosion
• Hydrodynamic simulations unravel the progenitor-supernova-remnant connection in SN 1987A
• 3D simulations of Rayleigh-Taylor mixing in core-collapse SNe with CASTRO
• Three-dimensional distribution of ejecta in Supernova 1987A at 10 000 days
• Aspherical Supernova Shock Breakout and the Observations of Supernova 2008D
• Supernova 1987A: neutrino-driven explosions in three dimensions and light curves
• The Three-Dimensional Structure of Interior Ejecta in Cassiopeia A at High Spectral Resolution
• 3D MHD modeling of the expanding remnant of SN 1987A. Role of magnetic field and non-thermal radio emission
• Emission line models for the lowest-mass core collapse supernovae. I: Case study of a 9 $M_{\odot }$ one-dimensional neutrino-driven explosion
• Gamma-Rays from Single Lobe Supernova Explosions
• Matter Mixing in Aspherical Core-collapse Supernovae: Three-dimensional Simulations with Single Star and Binary Merger Progenitor Models for SN 1987A
• Very Deep Inside the SN 1987A Core Ejecta: Molecular Structures Seen in 3D
• Dynamics of Fe-Ni Bubbles in Young Supernova Remnants
• Instabilities and Mixing in SN 1993J
• Light curve analysis of ordinary type IIP supernovae based on neutrino-driven explosion simulations in three dimensions
• A Case Study of Small Scale Structure Formation in 3D Supernova Simulations
• Three-dimensional mixing and light curves: constraints on the progenitor of supernova 1987A
• The Kinematic and Plasma Properties of X-ray Knots in Cassiopeia A from the Chandra HETGS
• The 30-Year Search for the Compact Object in SN 1987A
• Resolution Study for Three-dimensional Supernova Simulations with the Prometheus-Vertex Code
• The matter beyond the ring: the recent evolution of SN 1987A observed by the Hubble Space Telescope
• Erratum: Progenitor-explosion connection and remnant birth masses for neutrino-driven supernovae of iron-core progenitors (2012, ApJ, 757, 69)
• Asymmetry in the Outburst of SN 1987A Detected Using Light Echo Spectroscopy
• Non-spherical core collapse supernovae III. Evolution towards homology and dependence on the numerical resolution
• Properties of gamma-ray decay lines in 3D core-collapse supernova models, with application to SN 1987A and Cas A
• Matter mixing in aspherical core-collapse supernovae: a search for possible conditions for conveying ${}^{56}$Ni into high velocity regions
• X-Ray and Gamma-Ray Emission From Core-collapse Supernovae: Comparison of Three-dimensional Neutrino-driven Explosions With SN 1987A
• X-ray Absorption in Young Core-Collapse Supernova Remnants
• Clump Development by the Nickel Bubble Effect in Supernovae
• Spatial distribution of radionuclides in 3D models of SN 1987A and Cas A
• First Simulations of Core- Collapse Supernovae to Supernova Remnants with SNSPH

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